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| 001 | 618902 | ||
| 005 | 20250715171159.0 | ||
| 024 | 7 | _ | |a 10.1051/0004-6361/202348063 |2 doi |
| 024 | 7 | _ | |a 0004-6361 |2 ISSN |
| 024 | 7 | _ | |a 1432-0746 |2 ISSN |
| 024 | 7 | _ | |a arXiv:2401.07071 |2 arXiv |
| 024 | 7 | _ | |a WOS:001185071900015 |2 WOS |
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| 037 | _ | _ | |a PUBDB-2024-07224 |
| 041 | _ | _ | |a English |
| 082 | _ | _ | |a 520 |
| 088 | _ | _ | |a arXiv:2401.07071 |2 arXiv |
| 100 | 1 | _ | |a Aharonian, F. |b 0 |
| 245 | _ | _ | |a TeV flaring activity of the AGN PKS 0625–354 in November 2018 |
| 260 | _ | _ | |a Les Ulis |c 2024 |b EDP Sciences |
| 336 | 7 | _ | |a article |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
| 336 | 7 | _ | |a Journal Article |b journal |m journal |0 PUB:(DE-HGF)16 |s 1733221633_139311 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a JOURNAL_ARTICLE |2 ORCID |
| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 500 | _ | _ | |a 9 pages, 6 figures, accepted for publication in Astronomy & Astrophysics |
| 520 | _ | _ | |a Most γ-ray detected active galactic nuclei are blazars with one of their relativistic jets pointing towards the Earth. Only a few objects belong to theclass of radio galaxies or misaligned blazars. Here, we investigate the nature of the object PKS 0625−354, its γ-ray flux and spectral variabilityand its broad-band spectral emission with observations from H.E.S.S., Fermi-LAT, Swift-XRT, and UVOT taken in November 2018. The H.E.S.S.light curve above 200 GeV shows an outburst in the first night of observations followed by a declining flux with a halving time scale of 5.9 h. Theγγ-opacity constrains the upper limit of the angle between the jet and the line of sight to ∼10◦. The broad-band spectral energy distribution showstwo humps and can be well fitted with a single-zone synchrotron self Compton emission model. We conclude that PKS 0625−354, as an objectshowing clear features of both blazars and radio galaxies, can be classified as an intermediate active galactic nuclei. Multi-wavelength studiesof such intermediate objects exhibiting features of both blazars and radio galaxies are sparse but crucial for the understanding of the broad-bandemission of γ-ray detected active galactic nuclei in general |
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